One parameter that is well constrained by the gravitational waves detectors is the chirp mass \(\mathcal {M}_c\), which is a combination of the component masses of a binary neutron star system [1]}, [2]}
\(\mathcal {M}_c=\frac{(m_1m_2)^{3/5}}{(m_1+m_2)^{1/5}}=m_1\frac{q^{3/5}}{(1+q)^{1/5}},\) 
